Title: Toward detailed prominence seismology I. Computing accurate 2.5D magnetohydrodynamic equilibria
Authors: Blokland, J. W. S ×
Keppens, Rony #
Issue Date: Aug-2011
Publisher: EDP Sciences
Series Title: Astronomy & Astrophysics vol:532
Article number: A93
Abstract: Context. Prominence seismology exploits our knowledge of the linear eigenoscillations for representative magnetohydrodynamic models of filaments. To date, highly idealized models for prominences have been used, especially with respect to the overall magnetic configurations. Aims. We initiate a more systematic survey of filament wave modes, where we consider full multi-dimensional models with twisted magnetic fields representative of the surrounding magnetic flux rope. This requires the ability to compute accurate 2.5 dimensional magnetohydrodynamic equilibria that balance Lorentz forces, gravity, and pressure gradients, while containing density enhancements (static or in motion).
ISSN: 1432-0746
Publication status: published
KU Leuven publication type: IT
Appears in Collections:Plasma-astrophysics Section
× corresponding author
# (joint) last author

Files in This Item:

There are no files associated with this item.

Request a copy


All items in Lirias are protected by copyright, with all rights reserved.

© Web of science